{ "id": "1410.8539", "version": "v1", "published": "2014-10-30T20:06:58.000Z", "updated": "2014-10-30T20:06:58.000Z", "title": "Detection of Neutral Phosphorus in the Near Ultraviolet Spectra of Late-Type Stars", "authors": [ "Ian U. Roederer", "Heather R. Jacobson", "Thanawuth Thanathibodee", "Anna Frebel", "Elizabeth Toller" ], "comment": "Accepted for publication in the Astrophysical Journal. 13 pages, 4 figures", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "We report the detection of several absorption lines of neutral phosphorus (P, Z=15) in archival near ultraviolet spectra obtained with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. We derive phosphorus abundances or interesting upper limits in 14 late-type stars with metallicities spanning -3.8<[Fe/H]<-0.1. Previously, phosphorus had only been studied in Galactic stars with -1.0<[Fe/H]<+0.3. Iron lines reveal abundance offsets between the optical and ultraviolet regions, and we discuss and apply a correction factor to account for this offset. In stars with [Fe/H]>-1.0, the [P/Fe] ratio decreases toward the solar value with increasing metallicity, in agreement with previous observational studies. In stars with [Fe/H]<-1.0, <[P/Fe]>=+0.04+/-0.10, which overlaps with the [P/Fe] ratios found in several high-redshift damped Lyman-alpha systems. This behavior hints at a primary origin in massive stars.", "revisions": [ { "version": "v1", "updated": "2014-10-30T20:06:58.000Z" } ], "analyses": { "keywords": [ "late-type stars", "ultraviolet spectra", "neutral phosphorus", "space telescope imaging spectrograph", "high-redshift damped lyman-alpha systems" ], "publication": { "doi": "10.1088/0004-637X/797/1/69", "journal": "The Astrophysical Journal", "year": 2014, "month": "Dec", "volume": 797, "number": 1, "pages": 69 }, "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014ApJ...797...69R" } } }